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Titlebook: Solar History; An Introduction Claudio Vita-Finzi Book 2013 The Author(s) 2013 Cosmogenic istotopes.Global atmospheric circulation and jet

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Book 20139.99999% of the Sun’s existence – our knowledge of solar history depends largely on analogy with kindred main sequence stars, on the outcome of various kinds of modelling, and on indirect measures of solar activity. They include the analysis of lunar rocks and meteorites for evidence of solar flares
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2191-9100 ve monitored the Sun – that is to say for 99.99999% of the Sun’s existence – our knowledge of solar history depends largely on analogy with kindred main sequence stars, on the outcome of various kinds of modelling, and on indirect measures of solar activity. They include the analysis of lunar rocks
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Isotopes and Ice Cores,ciological reconstruction should eventually unlock the solar data inherent in .Be sequences that already span the last 800 kyr. There is also the promise of identifying solar energetic particle (SEP) events from nitrate-rich layers in ice cores.
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The Solar Cycle,f magnetic field lines by differential solar rotation; deeper links to internal dynamics are revealed by neutrino data. Periodicities which were not obvious when solar observation was limited to the photosphere may turn out to be more significant as regards the solar interior than the Schwabe or Hale cycle.
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Solar Rotation,od of 32 d it appears to lag behind the sunspot signal. An alternative explanation, for which there is support from periodicities in neutrino flux, is that, as once proposed by Dicke, the TSI is driven primarily by an internal ‘chronometer’.
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